一种改进的BDS三频单历元TCAR算法

针对原有TCAR算法中宽巷(WL)组合模糊度估计成功率不高的问题,该文通过分析BDS三频最优组合观测值性能,采用易于固定模糊度的超宽巷(EWL)组合代替原有TCAR法的宽巷组合,形成EWL+EWL+NL组合解算模式。在此基础上,对GB_TCAR法和改进的综合TCAR法的模糊度浮点解精度进行分析,并对实测BDS零基线、短基线和长基线数据进行模糊度解算。结果表明,GB_TCAR法和改进的综合TCAR法均可实现所有基线EWL组合模糊度的单历元可靠固定,且改进的综合TCAR法对模糊度解算有一定的改善作用,其中,对零基线、短基线NL组合模糊度的改善效果较明显,但随着基线长度增长,仍无法可靠地固定长基线NL组合模糊度。     

一种新的中长基线BDS三频模糊度快速解算方法

虽然TCAR能够实现短基线三频模糊度单历元解算,但由于电离层延迟及观测噪声等的影响,中长基线三频模糊度快速解算仍然是导航定位的一大难点。本文提出了一种新的无几何无电离层三频模糊度解算方法。该方法通过对伪距观测值赋予不同的权重,辅助宽巷及窄巷消除电离层残差的影响,使宽巷及窄巷求解只受观测噪声的影响;然后通过多历元的平滑获取宽巷及窄巷模糊度值。通过实测BDS三频长基线数据表明,相比经典TCAR算法,该方法可大大改善中长基线模糊度的求解精度,经过数据平滑并验证基本可以实现中长基线模糊度的快速解算。     

信噪比的GNSS宽巷模糊度单历元固定算法

针对常规GNSS解算模糊度存在的问题,该文提出了一种新的GNSS宽巷模糊度单历元求解算法。利用单历元双频码伪距观测值和载波相位观测值得到双差宽巷模糊度浮点解,将所有浮点宽巷模糊度分别向上、向下取整建立模糊度搜索空间;将模糊度空间中的所有备选组合代入双差宽巷观测方程中进行最小二乘解算,其中单位权中误差最小的组合就是最优的宽巷模糊度组合;然后对最优组合进行正确性检验以确定宽巷模糊度。确定宽巷模糊度后,可以利用宽巷观测值和载波观测值求出基础模糊度整周解。实验表明,该文提出的模糊度固定方法具有较高的成功率和可靠性,静态数据中模糊度固定成功率达到98.84%,动态数据中模糊度固定成功率达到了99.60%。     

信噪比的GNSS宽巷模糊度单历元固定算法

针对常规GNSS解算模糊度存在的问题,该文提出了一种新的GNSS宽巷模糊度单历元求解算法。利用单历元双频码伪距观测值和载波相位观测值得到双差宽巷模糊度浮点解,将所有浮点宽巷模糊度分别向上、向下取整建立模糊度搜索空间;将模糊度空间中的所有备选组合代入双差宽巷观测方程中进行最小二乘解算,其中单位权中误差最小的组合就是最优的宽巷模糊度组合;然后对最优组合进行正确性检验以确定宽巷模糊度。确定宽巷模糊度后,可以利用宽巷观测值和载波观测值求出基础模糊度整周解。实验表明,该文提出的模糊度固定方法具有较高的成功率和可靠性,静态数据中模糊度固定成功率达到98.84%,动态数据中模糊度固定成功率达到了99.60%。     

信噪比的GNSS宽巷模糊度单历元固定算法

针对常规GNSS解算模糊度存在的问题,该文提出了一种新的GNSS宽巷模糊度单历元求解算法。利用单历元双频码伪距观测值和载波相位观测值得到双差宽巷模糊度浮点解,将所有浮点宽巷模糊度分别向上、向下取整建立模糊度搜索空间;将模糊度空间中的所有备选组合代入双差宽巷观测方程中进行最小二乘解算,其中单位权中误差最小的组合就是最优的宽巷模糊度组合;然后对最优组合进行正确性检验以确定宽巷模糊度。确定宽巷模糊度后,可以利用宽巷观测值和载波观测值求出基础模糊度整周解。实验表明,该文提出的模糊度固定方法具有较高的成功率和可靠性,静态数据中模糊度固定成功率达到98.84%,动态数据中模糊度固定成功率达到了99.60%。     

零基线约束的参考站间模糊度固定方法研究

论文提出一种GNSS零基线约束的参考站间模糊度快速固定方法,该方法基于“一天线+双接收机”设计进行参考站间模糊度固定。首先,利用两个参考站四台接收机观测值形成四对参考站间无电离层组合双差观测值。其次,结合无电离层组合观测值模糊度和宽巷整周模糊度进行卡尔曼滤波和N1模糊度实数解计算。然后在模糊度域内进行线性变换,单历元固定零基线模糊度;利用零基线模糊度约束解算四组参考站间模糊度中的一组模糊度。最后,利用固定的模糊度还原所有原始双差整周模糊度。实验证明:与传统参考站间模糊度固定方法比,充分利用了零基线模糊度固定的约束条件进行参考站间模糊度固定,加快了模糊度收敛速度,极大地提高了模糊度固定的速度和成功率。      

信噪比的GNSS宽巷模糊度单历元固定算法

针对常规GNSS解算模糊度存在的问题,该文提出了一种新的GNSS宽巷模糊度单历元求解算法。利用单历元双频码伪距观测值和载波相位观测值得到双差宽巷模糊度浮点解,将所有浮点宽巷模糊度分别向上、向下取整建立模糊度搜索空间;将模糊度空间中的所有备选组合代入双差宽巷观测方程中进行最小二乘解算,其中单位权中误差最小的组合就是最优的宽巷模糊度组合;然后对最优组合进行正确性检验以确定宽巷模糊度。确定宽巷模糊度后,可以利用宽巷观测值和载波观测值求出基础模糊度整周解。实验表明,该文提出的模糊度固定方法具有较高的成功率和可靠性,静态数据中模糊度固定成功率达到98.84%,动态数据中模糊度固定成功率达到了99.60%。     

BDS/GPS组合单历元基线解算方法

阐述了BDS/GPS单历元解算函数模型的相关理论,并进行了相应的公式推导。在此基础上,利用基于正则化的载波相位解算模型,解算宽巷模糊度。首先将BDS卫星宽巷模糊度值作为约束固定出IGSO和MEO卫星的模糊度;然后再将IGSO和MEO卫星模糊度值作为约束来固定GEO卫星模糊度。通过实测数据对该方法进行测试和分析,结果表明:BDS/GPS组合系统单历元宽巷模糊度成功率为100%;基频模糊度成功率90%以上;N、E、U方向定位精度达到了毫米至厘米级。     

北斗三号新三频相位模糊度固定方法

针对北斗三号新的三频观测值,通过分析BDS-3三频线性组合观测值特性,选取高质量组合观测值,采用无几何相关GF(Geometry-Free)模型和无几何无电离层相关GIF(Geometry-Ionospheric-Free)模型分别对实测BDS-3卫星数据进行单历元三频相位模糊度解算TCAR(Triple-frequency Carrier Ambiguity Resolution)。试验结果表明,短基线时GF模型模糊度误差都在0.5周以内,且模糊度固定成功率都在88.43%以上;中长基线时GF模型模糊度固定能力明显降低,宽巷下降到73.47%,窄巷也只有25.44%。GIF模型在中长基线解算时相比于GF模型具有更好的模糊度固定能力。中长基线GIF模型宽巷模糊度固定成功率达85.31%,相对于GF模型提高了13%。中长基线GIF模型窄巷模糊度固定成功率在43.58%以上,相对于GF模型提高了51%。     

基于北斗三频的短基线单历元模糊度固定

采用三频观测值能组成更多波长更长、噪声较小的观测值;通过依次固定超宽巷、宽巷、窄巷模糊度,可以实现模糊度的快速固定。目前以TCAR、CIR为代表的方法均是基于无几何模型的方法,通过伪距直接求解相位模糊度;由于不同卫星模糊度各自单独求解,没有综合利用所有卫星的观测值信息。基于有几何模型,使用LAMBDA方法进行逐级模糊度固定,依次固定超宽巷、两个宽巷、两个无电离层组合窄巷模糊度,最后使用模糊度固定的两个无电离层组合进行最终基线解算。北斗实测数据验证表明,针对10km的短基线数据,采用本文方法可以实现100%的单历元模糊度固定的成功率。     

模糊度线性约束的消电离层多频模糊度解算

针对传统多频模糊度解算方法受到电离层延迟影响造成窄巷模糊度解算可靠性降低的问题,提出一种基于模糊度线性约束的消电离层MCAR方法。该方法通过模型等价性原理构建了基于几何相关-消电离层组合模型,并凭借能够可靠解算的超宽巷/宽巷模糊度值形成线性约束,进而构造窄巷模糊度解算模型,最终求解窄巷模糊度及精密定位结果。多组北斗三频实际数据测试结果表明,即使双差电离层延迟达到73.2 cm,所提出方法也可实现模糊度解算成功率高于96%,定位精度优于15 cm。     

基于LAMBDA和DC算法的GPS单历元整周模糊度的快速确定

仅利用LAMBDA方法求解GPS单历元整周模糊度成功率不高,并且当接收卫星数较多时搜索空间较大。为此,采用TIKHONOV正则化方法削弱单历元模型法方程的病态性,并且基于协方差矩阵选择部分宽巷模糊度,先采用LAMBDA方法进行搜索,再利用高解算效率的DC算法解算剩余宽巷模糊度,最后通过两组不同线性组合的逆变换直接求取原始观测值L1和L2的整周模糊度。实验和计算表明,方法显著提高整周模糊度的搜索效率,并且提高模糊度搜索成功率。     

Five-frequency Galileo long-baseline ambiguity resolution with multipath mitigation

For long-baseline over several hundreds of kilometers, the ionospheric delays that cannot be fully removed by differencing observations between receivers hampers rapid ambiguity resolution. Compared with forming ionospheric-free linear combination using dual- or triple-frequency observations, estimating ionospheric delays using uncombined observations keeps all the information of the observations and allows extension of the strategy to any number of frequencies. As the number of frequencies has increased for the various GNSSs, it is possible to study long-baseline ambiguity resolution performance using up to five frequencies with uncombined observations. We make use of real Galileo observations on five frequencies with a sampling interval of 1 s. Two long baselines continuously receiving signals from six Galileo satellites during corresponding test time intervals were processed to study the formal and empirical ambiguity success rates in case of full ambiguity resolution (FAR). The multipath effects are mitigated using the measurements of another day when the constellation repeats. Compared to the results using multipath-uncorrected Galileo observations, it is found that the multipath mitigation plays an important role in improving the empirical ambiguity success rates. A high number of frequencies are also found to be helpful to achieve high ambiguity success rate within a short time. Using multipath-uncorrected observations on two, three, four and five frequencies, the mean empirical success rates are found to be about 73, 88, 91, and 95% at 10 s, respectively, while the values are increased to higher than 86, 95, 98, and 99% after mitigating the multipath effects.     

URTK: undifferenced network RTK positioning

Standard network RTK has been widely used since it was proposed in the mid-1990s. Rovers can obtain high-precision estimates of position by resolving double-differenced (DD) ambiguities. The focus of this study is a new undifferenced network RTK method, abbreviated as URTK hereafter, based on undifferenced (UD) observation corrections whose single-differenced (SD) ambiguities between satellites can be resolved in several seconds. The tools for studying the real-time realization of the new method are our developments of logical schemes that have the capability for the real-time modeling of a reference network and the instantaneous resolution of SD ionosphere-free (IF) ambiguities at a single station. This research demonstrates the validity of modeling regional UD-unmodeled errors on the ground and examines the maximum differences when compared to modeling the errors using ionospheric pierce points (IPP). With data collected at 48 stations from a CORS network in Shanxi Province (SXCORS) in China through May 21, 2010, the efficiency of the presented real-time strategies is validated using IGS final products in a postprocessing mode. The results verify that more than 83 % of SD wide-lane (WL) ambiguity can be fixed with 5 s of observation data, and the average resolution time of all the WL tests is 4.96 s. More than 80 % of SD L1 ambiguity can be fixed within 5 s, and the average resolution time is only 6.66 s. Rovers could gain rapidly centimeter-level absolute positioning service, comparable to standard network RTK. In addition, the URTK method transforms the fixed DD-ambiguities of the reference network into UD-ambiguities, and it does not need to set the base station and base satellite. Since the UD-corrections are modeled for each common visible satellite, it breaks down the connections between stations and satellites of the DD-corrections in the current network RTK. The UD-corrections can be broadcast by the base station and automatically selected and optimized by a rover during the real-time kinematic processing, thus avoiding ambiguity in reinitialization due to the change of reference, so it should be very flexible and useful for a wide range of applications.     

北斗伪距码偏差对基线解算的影响分析

北斗二代系统伪距码中存在与高度角相关的系统性偏差,该偏差会影响高精度的数据处理。基于Melbourne-Wübbena（MW）组合,分别利用现有的伪距码偏差改正模型和实测基线的双差宽巷模糊度残差,分析了伪距码偏差对基线解算的影响。理论分析表明,随着基线长度的增加,伪距码偏差对MW组合确定双差宽巷模糊度的影响越来越大,对300 km基线的影响可达0.36周。实际算例表明,无论基线长短,地球同步轨道（geostationary earth orbit,GEO）卫星的双差宽巷模糊度残差中始终存在偏差;而对于倾斜地球同步轨道（inclined geostationary orbit,IGSO）和中轨（medium earth orbit,MEO）卫星而言,当基线小于300 km时,双差基本可以消除伪距码偏差,其双差宽巷模糊度固定率基本和GPS一致,但当基线超过300 km时,部分卫星的双差宽巷模糊度残差就会存在明显偏差,其双差宽巷模糊度固定率也较低,此时需考虑伪距码偏差的影响。     

航空测量场景下的中长基线动态定位方法

单基站中长基线动态相对定位受到大气残余误差影响，无法快速固定整周模糊度，定位精度和可靠性不如短基线场景。在航空测量场景下，流动站与基准站之间的基线由短到长变化，利用短基线场景下固定的整周模糊度反算得到高精度的电离层延迟量，并对其进行建模预报。随着基线变长，利用预报的电离层延迟约束中长基线定位模型，实现快速模糊度固定。本文分析了动态长基线情形下的电离层延迟的时变特性，采用滑动窗口进行电离层建模预报，讨论了该方法在航空测量实际作业中的实施条件、定位精度及模糊度固定情况。实测机载数据的解算结果表明，使用该方法，当测量载体出发阶段处于短基线场景下，单基站相对定位结果就可以达到接近100%的模糊度固定率，且定位精度保持在厘米级，显著减小了航空测量任务的作业成本。     

一种GPS整周模糊度单历元解算方法

仅利用单历元的载波相位观测值进行整周模糊度解算,观测方程秩亏,给单历元模糊度解算带来很大困难.因此,本文提出一种单历元确定GPS整周模糊度的方法.利用单历元测码伪距观测值和双频载波相位观测值组成双差观测方程,根据方差矩阵对宽巷模糊度进行分组,采用基于LABMDA方法的逐步解算方法来确定双差相位观测值的宽巷模糊度.确定宽...     

Triple-frequency GPS precise point positioning with rapid ambiguity resolution

At present, reliable ambiguity resolution in real-time GPS precise point positioning (PPP) can only be achieved after an initial observation period of a few tens of minutes. In this study, we propose a method where the incoming triple-frequency GPS signals are exploited to enable rapid convergences to ambiguity-fixed solutions in real-time PPP. Specifically, extra-wide-lane ambiguity resolution can be first achieved almost instantaneously with the Melbourne-Wübbena combination observable on L2 and L5. Then the resultant unambiguous extra-wide-lane carrier-phase is combined with the wide-lane carrier-phase on L1 and L2 to form an ionosphere-free observable with a wavelength of about 3.4 m. Although the noise of this observable is around 100 times the raw carrier-phase noise, its wide-lane ambiguity can still be resolved very efficiently, and the resultant ambiguity-fixed observable can assist much better than pseudorange in speeding up succeeding narrow-lane ambiguity resolution. To validate this method, we use an advanced hardware simulator to generate triple-frequency signals and a high-grade receiver to collect 1-Hz data. When the carrier-phase precisions on L1, L2 and L5 are as poor as 1.5, 6.3 and 1.5 mm, respectively, wide-lane ambiguity resolution can still reach a correctness rate of over 99 % within 20 s. As a result, the correctness rate of narrow-lane ambiguity resolution achieves 99 % within 65 s, in contrast to only 64 % within 150 s in dual-frequency PPP. In addition, we also simulate a multipath-contaminated data set and introduce new ambiguities for all satellites every 120 s. We find that when multipath effects are strong, ambiguity-fixed solutions are achieved at 78 % of all epochs in triple-frequency PPP whilst almost no ambiguities are resolved in dual-frequency PPP. Therefore, we demonstrate that triple-frequency PPP has the potential to achieve ambiguity-fixed solutions within a few minutes, or even shorter if raw carrier-phase precisions are around 1 mm. In either case, we conclude that the efficiency of ambiguity resolution in triple-frequency PPP is much higher than that in dual-frequency PPP.     

北斗三频电离层延迟及码硬件延迟解算方法

准确固定非差模糊度是利用相位观测量获取高精度电离层延迟的关键。三频观测条件下常规的处理策略需依次固定超宽巷、宽巷以及窄巷模糊度,通常利用MW（melbourne-wubbena）组合解算宽巷模糊度时易受到码硬件延迟和观测噪声的影响而固定错误。利用北斗三频数据和GIM（grid ionosphenimap）产品,通过固定的超宽巷模糊度以及构造相位无几何组合解算宽巷模糊度,进而重构得到高精度电离层延迟,并且分离了码硬件延迟总量。结果表明,GIM模型辅助条件下宽巷模糊度固定成功率能达到100%,且消除了系统性偏差;电离层重构值与GIM模型改正值存在约1 m的差异,等效精度约6TECU;分离的码硬件延迟变化平稳,标准偏差不超过0.3 m。